Great Eruption

Eta Carinae, formerly known as Eta Argus, is a stellar system containing at least two stars with a combined luminosity greater than five million times that of the Sun, located around 7,500 light-years distant in the constellation Carina. Previously a 4th-magnitude star, it brightened in 1837 to become brighter than Rigel, marking the start of its so-called "Great Eruption". It became the second-brightest star in the sky between 11 and 14 March 1843 before fading well below naked eye visibility after 1856. In a smaller eruption, it reached 6th magnitude in 1892 before fading again. It has brightened consistently since about 1940, becoming brighter than magnitude 4.5 by 2014. At declination −59° 41′ 04.26″, Eta Carinae is circumpolar from locations on Earth south of latitude 30°S,; and is not visible north of about latitude 30°N, just south of Cairo, which is at a latitude of 30°2′N. The two main stars of the Eta Carinae system have an eccentric orbit with a period of 5.54 years.

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What Caused Eta Carinae’s 1840 “Great Eruption?”

Chandra Discovers New Details about ‘Great Eruption’ of Eta Carinae

Astronomers rewind the clock on Eta Carinae’s “Great Eruption” of 1837, showing in a new paper that the X-ray power alone released by the explosion was about 10 million times greater than the entire radiant power of the Sun across all wavelengths.